Notice: As of 4:26 p.m. EDT,
the GOES-16 ABI Imager (GOES-East) is offline due to a reported thermal anomaly.
No GOES-East images will be updated while the satellite is offline.
As soon as data flow is restored, we will begin processing images and update the site.
GOES-West continues to operate normally.
30 May 2024 - 07:07 EDT
30 May 2024 - 11:07 UTC
Post-tropical Cyclone Laura - Nighttime Microphysics at 38.4°N - 83.3°W
To enlarge, pause animation & click the image. Hover over popups to zoom. Use slider to navigate. Apparent 'jumps' in the animation occur due to adjustments to reflect storm movement.
While GOES animation code will not run on older Internet Explorer browsers,
they work in the newest versions of Microsoft Edge. If you are using
Internet Explorer, please try a different browser: Chrome, Firefox, Safari, or
MS Edge are all supported.
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1200 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1210 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1220 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1230 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1250 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1300 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1320 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1330 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1340 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1350 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1400 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1410 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1420 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1430 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1440 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1450 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1520 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1530 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1540 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1550 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1610 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1620 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1630 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 29 Aug 2020 - 1650 UTC
This RGB will be phased out around 1 Feb 2023 and will be replaced by the Day Night Cloud Micro Combo RGB.
Nighttime Microphysics RGB The distinction between low clouds and fog in satellite imagery is challenging. While the difference between the 10.4 and 3.9 μm channels has been a regularly applied product to meet aviation forecast needs, the Nighttime Microphysics (NtMicro) RGB adds another channel difference (12.4- 10.4 μm) as a proxy to cloud thickness and repeats the use of the 10.4 μm thermal channel to enhance areas of warm (i.e. low) clouds where fog is more likely. The NtMicro RGB is also an efficient tool to quickly identify other cloud types in the mid and upper atmosphere.